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<ri:Resource created="2018-11-27T13:26:36Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Properties of variables in the NGC 1846 field</title><shortName>J/AJ/155/183</shortName><identifier>ivo://CDS.VizieR/J/AJ/155/183</identifier><altIdentifier>doi:10.26093/cds/vizier.51550183</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Salinas R.</name></creator><creator><name>Pajkos M.A.</name></creator><creator><name>Vivas A.K.</name></creator><creator><name>Strader J.</name></creator><creator><name>Contreras Ramos R.</name></creator><date role="Updated">2020-01-31T11:57:45Z</date><date role="Created">2018-11-27T13:26:36Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>magellanic-clouds</subject><subject>globular-star-clusters</subject><subject>variable-stars</subject><subject>visible-astronomy</subject><subject>sloan-photometry</subject><subject>astronomical-object-identification</subject><description>Intermediate-age (IA) star clusters in the Large Magellanic Cloud (LMC) present extended main-sequence turn-offs (MSTO) that have been attributed to either multiple stellar populations or an effect of stellar rotation. Recently it has been proposed that these extended main sequences can also be produced by ill-characterized stellar variability. Here we present Gemini-S/Gemini Multi-Object Spectrometer (GMOS) time series observations of the IA cluster NGC 1846. Using differential image analysis, we identified 73 new variable stars, with 55 of those being of the Delta Scuti type, that is, pulsating variables close the MSTO for the cluster age. Considering completeness and background contamination effects, we estimate the number of {delta} Sct belonging to the cluster between 40 and 60 members, although this number is based on the detection of a single {delta} Sct within the cluster half-light radius. This amount of variable stars at the MSTO level will not produce significant broadening of the MSTO, albeit higher-resolution imaging will be needed to rule out variable stars as a major contributor to the extended MSTO phenomenon. Though modest, this amount of {delta} Sct makes NGC 1846 the star cluster with the highest number of these variables ever discovered. Lastly, our results present a cautionary tale about the adequacy of shallow variability surveys in the LMC (like OGLE) to derive properties of its {delta} Sct population.</description><source format="bibcode">2018AJ....155..183S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/155/183</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/53/93">J/AcA/53/93 : OGLE RR Lyrae in LMC (Soszynski+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/59/1">J/AcA/59/1 : VI light curves of LMC RR Lyrae stars (Soszynski+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/59/239">J/AcA/59/239 : VI light curves of LMC long-period variables</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/60/1">J/AcA/60/1 : VI light curves of LMC delta Scuti stars (Poleski+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/145/160">J/AJ/145/160 : Variables in LMC globular clusters. III. Reticulum</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/430/676">J/MNRAS/430/676 : Massive clusters in the LMC (Baumgardt+, 2013)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/155/183</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/155/183</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/155/183</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/155/183</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/155/183</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/155/183</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/AJ/155/183/table1 (Positions, mean magnitudes, r amplitudes, periods and classification for all of the variables discovered in the NGC 1846 field)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/155/183/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/155/183/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/155/183/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>76.79192083</ra><dec>-67.47620833</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/33124</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/155/183?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/AJ/155/183/table1</name><description>Positions, mean magnitudes, r amplitudes, periods and classification for all of the variables discovered in the NGC 1846 field</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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